Note on counterterms in asymptotically flat spacetimes

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dc.creatorAstefanesei, Dumitru
dc.creatorMann, Robert B.
dc.creatorStelea, Cristian
dc.date2006-08-04
dc.date2006-08-17
dc.date.accessioned2026-07-07T10:26:01Z
dc.date.available2026-07-07T10:26:01Z
dc.descriptionWe consider in more detail the covariant counterterm proposed by Mann and Marolf in asymptotically flat spacetimes. With an eye to specific practical computations using this counterterm, we present explicit expressions in general $d$ dimensions that can be used in the so-called `cylindrical cut-off' to compute the action and the associated conserved quantities for an asymptotically flat spacetime. As applications, we show how to compute the action and the conserved quantities for the NUT-charged spacetime and for the Kerr black hole in four dimensions.
dc.description13 pages, v. 2 added references
dc.identifierhttps://arxiv.org/abs/hep-th/0608037
dc.identifierhttp://arxiv.org/abs/hep-th/0608037
dc.identifierPhys.Rev.D75:024007,2007
dc.identifierdoi:10.1103/PhysRevD.75.024007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176736
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNote on counterterms in asymptotically flat spacetimes
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